"Parking-garage" structures in nuclear astrophysics and cellular biophysics

被引:49
作者
Berry, D. K. [1 ,2 ]
Caplan, M. E. [1 ,2 ]
Horowitz, C. J. [1 ,2 ]
Huber, Greg [3 ]
Schneider, A. S. [4 ]
机构
[1] Indiana Univ, Ctr Explorat Energy & Matter, Bloomington, IN 47405 USA
[2] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA
[3] Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Kohn Hall, Santa Barbara, CA 93106 USA
[4] CALTECH, Walter Burke Inst Theoret Phys, TAPIR, MC 350-17, Pasadena, CA 91125 USA
基金
美国国家科学基金会;
关键词
NEUTRON-STAR; CRUST;
D O I
10.1103/PhysRevC.94.055801
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
A striking shape was recently observed for the endoplasmic reticulum, a cellular organelle consisting of stacked sheets connected by helical ramps [Terasaki et al., Cell 154, 285 ( 2013)]. This shape is interesting both for its biological function, to synthesize proteins using an increased surface area for ribosome factories, and its geometric properties that may be insensitive to details of the microscopic interactions. In the present work, we find very similar shapes in our molecular dynamics simulations of the nuclear pasta phases of dense nuclear matter that are expected deep in the crust of neutron stars. There are dramatic differences between nuclear pasta and terrestrial cell biology. Nuclear pasta is 14 orders of magnitude denser than the aqueous environs of the cell nucleus and involves strong interactions between protons and neutrons, while cellular-scale biology is dominated by the entropy of water and complex assemblies of biomolecules. Nonetheless, the very similar geometry suggests both systems may have similar coarse-grained dynamics and that the shapes are indeed determined by geometrical considerations, independent of microscopic details. Many of our simulations self-assemble into flat sheets connected by helical ramps. These ramps may impact the thermal and electrical conductivities, viscosity, shear modulus, and breaking strain of neutron star crust. The interaction we use, with Coulomb frustration, may provide a simple model system that reproduces many biologically important shapes.
引用
收藏
页数:5
相关论文
共 27 条
  • [1] Effect of Coulomb screening length on nuclear "pasta" simulations
    Alcain, P. N.
    Gimenez Molinelli, P. A.
    Nichols, J. I.
    Dorso, C. O.
    [J]. PHYSICAL REVIEW C, 2014, 89 (05):
  • [2] The R-MODE instability in rotating neutron stars
    Andersson, N
    Kokkotas, KD
    [J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2001, 10 (04): : 381 - 441
  • [4] Caplan M. E., ARXIV160603646
  • [5] Topological characterization of neutron star crusts
    Dorso, C. O.
    Gimenez Molinelli, P. A.
    [J]. PHYSICAL REVIEW C, 2012, 86 (05):
  • [6] ON THE NUCLEAR CURVATURE ENERGY
    DURAND, M
    SCHUCK, P
    VINAS, X
    [J]. ZEITSCHRIFT FUR PHYSIK A-HADRONS AND NUCLEI, 1993, 346 (02): : 87 - 100
  • [7] Terasaki Spiral Ramps in the Rough Endoplasmic Reticulum
    Guven, Jemal
    Huber, Greg
    Maria Valencia, Dulce
    [J]. PHYSICAL REVIEW LETTERS, 2014, 113 (18)
  • [8] SHAPE OF NUCLEI IN THE CRUST OF NEUTRON STAR
    HASHIMOTO, M
    SEKI, H
    YAMADA, M
    [J]. PROGRESS OF THEORETICAL PHYSICS, 1984, 71 (02): : 320 - 326
  • [9] ELASTIC PROPERTIES OF LIPID BILAYERS - THEORY AND POSSIBLE EXPERIMENTS
    HELFRICH, W
    [J]. ZEITSCHRIFT FUR NATURFORSCHUNG C-A JOURNAL OF BIOSCIENCES, 1973, C 28 (11-1): : 693 - 703
  • [10] Disordered Nuclear Pasta, Magnetic Field Decay, and Crust Cooling in Neutron Stars
    Horowitz, C. J.
    Berry, D. K.
    Briggs, C. M.
    Caplan, M. E.
    Cumming, A.
    Schneider, A. S.
    [J]. PHYSICAL REVIEW LETTERS, 2015, 114 (03)